DARTS/Astro Query System - SQL Search -

All the tables available for SQL Search and information on each table are listed in the Available Data page. Please see the User Guide for the usage of "SQL Search".

total 1

No.
object_name
center_ra
center_dec
center_ra_b1950
center_dec_b1950
center_ecliptic_lon
center_ecliptic_lat
center_galactic_lon
center_galactic_lat
roll_angle
observation_start_time_mjd
observation_start_time
observation_end_time_mjd
observation_end_time
observation_id
exposure
awarded_exposure
xis0_exposure
xis1_exposure
xis2_exposure
xis3_exposure
xis0_observation_mode
xis1_observation_mode
xis2_observation_mode
xis3_observation_mode
hxd_observation_mode
hxd_coarse_clock_rate_exposure
hxd_first_clock_rate_exposure
hxd_normal_clock_rate_exposure
hxd_all_clock_rate_exposure
hxd_wam_exposure
quantity_of_hxd_burst
processing_status
processing_date_mjd
processing_date
public_date_mjd
public_date
distribution_date_mjd
distribution_date
processing_version
processing_count
processing_software
proposal_id
proposal_abstract
proposal_category
proposal_category_code
proposal_priority
pi_name
co_pi_name
proposal_affiliated_country
proposal_cycle
observation_type
proposal_title
main_instrument
has_xis_injection
data_access_url
ql_access_url
ql_image_url
1 CIZA J2242.8+5301 340.7602 53.1616 340.242904 52.89922 13.612188 54.382245 104.28022824 -4.9963098 17.994 55770.5553703704 2011-07-28 13:19:44 55772.8210185185 2011-07-30 19:42:16 806001010 122.9419 120 122.9499 122.9499 0 122.9419 2 2 0 2 1 0 0 134.8043 134.8043 195.7079 1 PROCESSED 57602.7365393518 2016-08-02 17:40:37 56162 2012-08-23 00:00:00 55792.3410069445 2011-08-19 08:11:03 3.0.22.44 2 Hea_08Feb2016_V6.18_Suzaku_14Nov2013_V22 060014 Radio relics in merging clusters have been considered to be synchrotron emission at a shock front. Nevertheless, no concrete evidence of the connection between relics and shocks has been unveiled yet. We propose a SUZAKU observation of a giant radio relic in a new merging cluster CIZA J2242.8+5301 recently discovered. Temperature and density maps across the giant radio relic will provide a clear illustration of the shock structure or a strong constraint of an origin of the radio relic. EXTRAGALACTIC DIFFUSE SOURCES 8 A HAJIME KAWAHARA SHO NISHINO JAP 6 AO6 SUZAKU OBSERVATION OF A NEW MERGING CLUSTER WITH A GIANT RADIO RELIC XIS Y https://data.darts.isas.jaxa.jp/pub/suzaku/ver3.0/806001010/ Quick Look

Used SQL

SELECT * FROM suzaku_master_data WHERE observation_id = '806001010'

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